Direct and fast calculation of regularized cosmological power spectrum at two-loop order
暂无分享,去创建一个
[1] E. Komatsu,et al. EXTRACTING ANGULAR DIAMETER DISTANCE AND EXPANSION RATE OF THE UNIVERSE FROM TWO-DIMENSIONAL GALAXY POWER SPECTRUM AT HIGH REDSHIFTS: BARYON ACOUSTIC OSCILLATION FITTING VERSUS FULL MODELING , 2008, 0805.4238.
[2] T. Matsubara. Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture , 2008, 0807.1733.
[3] Martin White,et al. Critical look at cosmological perturbation theory techniques , 2009, 0905.0479.
[4] Yong-Seon Song,et al. Reconstructing the history of structure formation using redshift distortions , 2008, 0807.0810.
[5] M. Crocce,et al. Memory of initial conditions in gravitational clustering , 2006 .
[6] A. Taruya,et al. Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations , 2011, 1106.4562.
[7] S. Matarrese,et al. Resumming cosmic perturbations , 2007, astro-ph/0703563.
[8] F. Bernardeau,et al. Constructing regularized cosmic propagators , 2011, 1112.3895.
[9] M. Crocce,et al. Renormalized cosmological perturbation theory , 2006 .
[10] Takahiro Nishimichi,et al. Nonlinear evolution of baryon acoustic oscillations from improved perturbation theory in real and redshift spaces , 2009, 0906.0507.
[11] Y. Jing,et al. Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of $N$-body Simulations and Analytic Models , 2008, 0810.0813.
[12] T. Matsubara,et al. Next-to-leading resummation of cosmological perturbations via the Lagrangian picture: 2-loop correction in real and redshift spaces , 2011, 1105.1491.
[13] F. Bernardeau,et al. Multipoint propagators for non-Gaussian initial conditions , 2010, 1006.4656.
[14] M. Bartelmann,et al. Weak gravitational lensing , 2016, Scholarpedia.
[15] F. Bernardeau,et al. Resummed propagators in multi-component cosmic fluids with the eikonal approximation , 2011, 1109.3400.
[16] M. Crocce,et al. Nonlinear evolution of baryon acoustic oscillations , 2007, 0704.2783.
[17] Thomas Hahn,et al. Cuba - a library for multidimensional numerical integration , 2004, Comput. Phys. Commun..
[18] H. Hoekstra,et al. Very weak lensing in the CFHTLS Wide: Cosmology from cosmic shear in the linear regime , 2007, 0712.0884.
[19] S. Colombi,et al. Large scale structure of the universe and cosmological perturbation theory , 2001, astro-ph/0112551.
[20] N. Padmanabhan,et al. Constraining anisotropic baryon oscillations , 2008, 0804.0799.
[21] Takahiro Sato,et al. Testing General Relativity with the Multipole Spectra of the SDSS Luminous Red Galaxies , 2008, 0805.4789.
[22] P. Valageas. A new approach to gravitational clustering: A path-integral formalism and large-N expansions , 2004 .
[23] E. Linder. Redshift distortions as a probe of gravity , 2007, 0709.1113.
[24] Earl Lawrence,et al. THE COYOTE UNIVERSE. III. SIMULATION SUITE AND PRECISION EMULATOR FOR THE NONLINEAR MATTER POWER SPECTRUM , 2009, 0912.4490.
[25] M. Pietroni,et al. Flowing with time: a new approach to non-linear cosmological perturbations , 2008, 0806.0971.
[26] A. Mazure,et al. A test of the nature of cosmic acceleration using galaxy redshift distortions , 2008, Nature.
[27] Patrick McDonald. Dark matter clustering: a simple renormalization group approach , 2007 .
[28] P. Schneider,et al. Detection of correlated galaxy ellipticities on CFHT data: first evidence for gravitational lensing by large-scale structures , 2000, astro-ph/0002500.
[29] S. Saito,et al. Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory , 2010, 1006.0699.
[30] Edward J. Wollack,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE * OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.
[31] F. Bernardeau,et al. Multipoint propagators in cosmological gravitational instability , 2008, 0806.2334.
[32] T. Matsubara,et al. Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space , 2007, 0711.2521.
[33] T. Nishimichi,et al. Combining perturbation theories with halo models , 2010, 1009.0597.
[34] P. Valageas. Large-N expansions applied to gravitational clustering , 2006, astro-ph/0611849.
[35] R. Smith,et al. Motion of the Acoustic Peak in the Correlation Function , 2007, astro-ph/0703620.
[36] K. Izumi,et al. Renormalized Newtonian cosmic evolution with primordial non-Gaussianity , 2007, 0706.1604.